On the cosmological gravitational waves and cosmological distances
V.A. Belinski, G.V. Vereshchagin
TL;DR
This paper explores how solitonic gravitational waves in the early universe could influence cosmological distance measurements, potentially affecting our understanding of the universe's expansion.
Contribution
It introduces a novel mechanism by which early universe gravitational waves can alter cosmological distances, linking inhomogeneities to observable effects.
Findings
Solitonic gravitational waves can propagate through the Friedmann universe.
These waves may cause an increase in cosmological distances.
The mechanism connects early universe inhomogeneities to observable cosmological phenomena.
Abstract
We show that solitonic cosmological gravitational waves propagated through the Friedmann universe and generated by the inhomogeneities of the gravitational field near the Big Bang can be responsible for increase of cosmological distances.
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